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Paper Citation Record · LEDGER

The Second Data Release of the Sloan Digital Sky Survey

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0403325.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/0403325 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:30:01.674745Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-06-27T11:00:51.336985Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e7b8d742-2271-44b5-9dc2-fa2419461b23 · inbound

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy cites this paper.

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy The Second Data Release of the Sloan Digital Sky Survey

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-14T14:30:01.674745Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:30:01.674745Z digest=sha256:6f1744cce53390cdf1ec240d28dd5d770c3af547b73c63f012e7299f9b6633a5

Observation 767c21f8-1629-4f64-b641-0836d4aed569 · inbound

Continuum optical-UV and X-ray variability of AGN: current results and future challenges cites this paper.

Continuum optical-UV and X-ray variability of AGN: current results and future challenges The Second Data Release of the Sloan Digital Sky Survey

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-06T21:45:07.475318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T21:45:07.475318Z digest=sha256:5e506ef49d1ba4be91c6efe45998e392bdcf7d0d72e2ee7d26ec30cb7137e8ae

Observation c0933f3c-4efc-493d-942a-84810e2c9b3c · inbound

Recalibration of SDSS photometric zero-points based on the InfraRed Flux Method temperature scale cites this paper.

Recalibration of SDSS photometric zero-points based on the InfraRed Flux Method temperature scale The Second Data Release of the Sloan Digital Sky Survey

Reference 8

Resolution
verified exact
local_arxiv, observed 2026-06-27T11:00:51.338469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bca659cd76ad64595e95dec8f3f70601fba454933cb45fc48bb0797b02c1c5ff

Observation b7f8e221-f69d-4bfd-9e19-f41ef0f87505 · inbound

Empirical colour--effective temperature relations in the SDSS system from IRFM temperatures of GALAH and APOGEE stars cites this paper.

Empirical colour--effective temperature relations in the SDSS system from IRFM temperatures of GALAH and APOGEE stars The Second Data Release of the Sloan Digital Sky Survey

Reference 11

Resolution
verified exact
local_arxiv, observed 2026-06-27T10:40:50.609033Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e0e77226e13661154d0cf0ae05cc5968209137ab26451e52ed50eb54d2f9272c

Observation 0b108b1d-dea6-40ca-99e2-79e8a029e6cf · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Second Data Release of the Sloan Digital Sky Survey

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:59:08.892503Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:022dc2b94190d8875e1882b8050eb17f25bae92e2e2b6f63f493b333cb20fefd